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A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants

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Iyudin,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Obergaulinger, M., Chimeno, J., Mimica, P., Aloy, M., & Iyudin, A. (2015). A method for computing synchrotron and inverse-Compton emission from hydrodynamic simulations of supernova remnants. High Energy Density Physics, 17, Part A Special Issue, 92-97.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0029-57E9-7
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